SDO HMI 2014-04-07 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.56 | 0.00 | 12.37 | -9.21 | 8.18 | 9.44 | 248.42 | 0.1785 | 252.5 | 337.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.82 | 0.00 | 1.44 | -8.14 | 12.90 | 14.16 | 261.11 | 0.2462 | 415.0 | 614.9 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -8.37 | 12.31 | 13.57 | 259.86 | 0.2370 | 775.0 | 626.4 | |
| 0.00 | 2.64 | 0.00 | 1.34 | -9.10 | 10.66 | 11.92 | 255.28 | 0.2118 | 1031.0 | 827.6 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -8.86 | 10.49 | 11.75 | 256.22 | 0.2082 | 896.0 | 693.1 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -9.23 | 10.20 | 11.46 | 254.16 | 0.2047 | 951.0 | 766.0 | |
| 0.00 | 4.49 | 0.00 | 2.26 | -10.49 | 8.47 | 9.73 | 245.12 | 0.1840 | 615.0 | 699.5 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -10.30 | 7.26 | 8.52 | 243.28 | 0.1639 | 882.0 | 677.5 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -7.39 | 6.49 | 7.75 | 260.42 | 0.1363 | -933.0 | -739.6 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -6.85 | 6.45 | 7.71 | 264.37 | 0.1345 | -794.0 | -649.5 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -7.07 | 5.88 | 7.14 | 262.24 | 0.1250 | -1214.0 | -958.7 | |
| 0.00 | 2.03 | 0.00 | 1.01 | -7.62 | 5.52 | 6.78 | 257.37 | 0.1205 | -1001.0 | -919.1 | |
| 0.00 | 1.67 | 0.00 | 0.84 | -11.69 | 4.12 | 5.38 | 223.46 | 0.1341 | 870.0 | 708.8 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -12.64 | 358.87 | 0.13 | 181.14 | 0.1135 | 789.0 | 701.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |